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Erosion Rates on Mars and Implications for Climate Change: Constraints From the Pathfinder Landing Site
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| dc.contributor.author | Golombek, M. | en_US |
| dc.contributor.author | Bridges, N. | en_US |
| dc.date.accessioned | 2004-09-24T16:33:35Z | |
| dc.date.available | 2004-09-24T16:33:35Z | |
| dc.date.issued | 1999 | en_US |
| dc.identifier.citation | Journal of Geophysical Research, Planets | en_US |
| dc.identifier.citation | USA | en_US |
| dc.identifier.clearanceno | 99-1338 | en_US |
| dc.identifier.uri | http://hdl.handle.net/2014/17888 | |
| dc.description.abstract | The observation that the Mars Pathfinder landing site looks very similar to its apperance after it was deposited by catastrophic floods some 1.8-3.5 Ga allows quantitative constraints to be placed on the rate of change of the site since that time. | en_US |
| dc.format.extent | 3013575 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en_US | |
| dc.subject.other | Erosion Mars Climate change | en_US |
| dc.title | Erosion Rates on Mars and Implications for Climate Change: Constraints From the Pathfinder Landing Site | en_US |
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JPL TRS 1992+
JPL TRS 1992+